Earth’s Ocean And Beyond

Earth’s Ocean and Beyond

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Image Credit: NOAA

Earth’s ocean has been the backdrop for ancient epics, tales of fictional fish and numerous scientific discoveries. It was, and will always be, a significant piece of the Earth’s story. Most of the ocean is unexplored– about 95% of this underwater realm is unseen by human eyes (NOAA). There is only one global Ocean. In fact, the ocean represents over 70% of the Earth’s surface and contains 96.5% of the Earth’s water.

We and the NOAA Office of Ocean Exploration and Research work together alongside organizations like the Schmidt Ocean Institute and Ocean Exploration Trust to better understand our oceans and its processes. While space may be the final frontier, understanding our own planet helps scientists as they explore space and study how our universe came to be.

On #WorldOceansDay let’s explore how Earth’s ocean informs our research throughout the solar system.

Earth and Exoplanets

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“In interpreting what we see elsewhere in the solar system and universe, we always compare with phenomena that we already know of on Earth…We work from the familiar toward the unknown.” - Norman Kuring, NASA Goddard

We know of only one living planet: our own. As we move to the next stage in the search for alien life, the effort will require the expertise of scientists of all disciplines. However, the knowledge and tools NASA has developed to study life on Earth will also be one of the greatest assets to the quest.

The photo above shows what Earth would look like at a resolution of 3 pixels, the same that exoplanet-discovering missions would see. What should we look for, in the search of other planets like our own? What are the unmistakable signs of life, even if it comes in a form we don’t fully understand? Liquid water; every cell we know of – even bacteria around deep-sea vents that exist without sunlight – requires water.

Phytoplankton (Algae) Bloom vs. Atmosphere of Jupiter

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Jupiter’s storms are mesmerizing in their beauty, captured in many gorgeous photos throughout the decades from missions like Voyager 1 and Juno. The ethereal swirls of Jupiter are the result of fluids in motion on a rotating body, which might come as a surprise, since its atmosphere is made of gas!

The eddies in Jupiter’s clouds appear very similar to those found in Earth’s ocean, like in the phytoplankton (or algae) bloom in the Baltic Sea, pictured above. The bloom was swept up in a vortex, just a part of how the ocean moves heat, carbon, and nutrients around the planet. Blooms like this, however, are not all beauty - they create “dead zones” in the areas where they grow, blooming and decaying at such a high rate that they consume all the oxygen in the water around them.

Arctic Sea Ice and Europa Ice Crust

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While the Arctic (North Pole) and the Antarctic (South Pole) are “polar opposites,” there is one huge difference between the North and South Poles– land mass. The Arctic is ocean surrounded by land, while the Antarctic is land surrounded by ocean. The North Pole  is located in the middle of the Arctic Ocean amid waters that are almost permanently covered with constantly shifting sea ice.

By studying this sea ice, scientists can research its impact on Earth system and even formation processes on other bodies like Europa, an icy moon of Jupiter. For example, it is possible that the reddish surface features on Europa’s ice may have communicated with a global subsurface ocean layer during or after their formation. 

Aquanauts and Astronauts

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As new missions are being developed, scientists are using Earth as a testbed. Just as prototypes for our Mars rovers made their trial runs on Earth’s deserts, researchers are testing both hypotheses and technology on our oceans and extreme environments.

NEEMO, our Extreme Environment Mission Operations project, is an analog mission that sends groups of astronauts, engineers and scientists to live in Aquarius, the world’s only undersea research station located off the Florida Keys, 62 feet (19 meters) below the surface. Much like space, the undersea world is a hostile, alien place for humans to live. NEEMO crew members, known as aquanauts, experience some of the same challenges there that they would on a distant asteroid, planet or moon.

Deep-sea Robotic Exploration and Space Robotic Exploration

Earth’s Ocean And Beyond

Video credit: Deep Sea Robotics/Schmidt Ocean Institute and Mars Curiosity rover/NASA

From mapping the seafloor through bathymetry to collecting samples on the surface of Mars, researchers are utilizing new technologies more than ever to explore. Satellite and robotic technology allow us to explore where humans may not be able to– yet. They teach us valuable lessons about the extreme and changing environments, science, as well as provide a platform to test new technologies.

Jezero Crater and Dvina River Delta, Arkhangelsk, Russia/Mars Delta

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River deltas, the point where a river meets the ocean, are sites of rich sediment and incredible biodiversity. The nutrients that rivers carry to the coastlines make a fertile place for fish and shellfish to lay their eggs.

The Jezero crater on Mars (pictured in false-color on the right) has been selected as the Mars2020 landing site, and has a structure that looks much like a river delta here on Earth! Pictures from our Mars Global Surveyor orbiter show eroded ancient deposits of transported sediment long since hardened into interweaving, curved ridges of layered rock. This is one of many hints that Mars was once covered in an ancient ocean that had more water than the Arctic Ocean. Studying these deltas on Earth helps us spot them on other planets, and learning about the ocean that was once on Mars informs how our own formed.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

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6 years ago
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A New Chandra Image Shows The Location Of Several Elements Produced By The Explosion Of A Massive Star.
A New Chandra Image Shows The Location Of Several Elements Produced By The Explosion Of A Massive Star.
A New Chandra Image Shows The Location Of Several Elements Produced By The Explosion Of A Massive Star.

A new Chandra image shows the location of several elements produced by the explosion of a massive star.

Cassiopeia A is a well-known supernova remnant located about 11,000 light years from Earth.

Supernova remnants and the elements they produce are very hot — millions of degrees — and glow strongly in X-ray light.

Chandra’s sharp X-ray vision allows scientists to determine both the amount and location of these crucial elements objects like Cas A produce.

Where do most of the elements essential for life on Earth come from? The answer: inside the furnaces of stars and the explosions that mark the end of some stars’ lives.Astronomers have long studied exploded stars and their remains — known as “supernova remnants” — to better understand exactly how stars produce and then disseminate many of the elements observed on Earth, and in the cosmos at large.Due to its unique evolutionary status, Cassiopeia A (Cas A) is one of the most intensely studied of these supernova remnants. A new image from NASA’s Chandra X-ray Observatory shows the location of different elements in the remains of the explosion: silicon (red), sulfur (yellow), calcium (green) and iron (purple). Each of these elements produces X-rays within narrow energy ranges, allowing maps of their location to be created. The blast wave from the explosion is seen as the blue outer ring.

X-ray telescopes such as Chandra are important to study supernova remnants and the elements they produce because these events generate extremely high temperatures — millions of degrees — even thousands of years after the explosion. This means that many supernova remnants, including Cas A, glow most strongly at X-ray wavelengths that are undetectable with other types of telescopes.Chandra’s sharp X-ray vision allows astronomers to gather detailed information about the elements that objects like Cas A produce. For example, they are not only able to identify many of the elements that are present, but how much of each are being expelled into interstellar space.

Much more reading/info/video:  http://chandra.harvard.edu/photo/2017/casa_life/

7 years ago

What are the Universe’s Most Powerful Particle Accelerators?

Every second, every square meter of Earth’s atmosphere is pelted by thousands of high-energy particles traveling at nearly the speed of light. These zippy little assailants are called cosmic rays, and they’ve been puzzling scientists since they were first discovered in the early 1900s. One of the Fermi Gamma-ray Space Telescope’s top priority missions has been to figure out where they come from.

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“Cosmic ray” is a bit of a misnomer. Makes you think they’re light, right? But they aren’t light at all! They’re particles that mostly come from outside our solar system — which means they’re some of the only interstellar matter we can study — although the Sun also produces some. Cosmic rays hit our atmosphere and break down into secondary cosmic rays, most of which disperse quickly in the atmosphere, although a few do make it to Earth’s surface.

Cosmic rays aren’t dangerous to those of us who spend our lives within Earth’s atmosphere. But if you spend a lot of time in orbit or are thinking about traveling to Mars, you need to plan how to protect yourself from the radiation caused by cosmic rays.

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Cosmic rays are subatomic particles — smaller particles that make up atoms. Most of them (99%) are nuclei of atoms like hydrogen and helium stripped of their electrons. The other 1% are lone electrons. When cosmic rays run into molecules in our atmosphere, they produce secondary cosmic rays, which include even lighter subatomic particles.

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Most cosmic rays reach the same amount of energy a small particle accelerator could produce. But some zoom through the cosmos at energies 40 million times higher than particles created by the world’s most powerful man-made accelerator, the Large Hadron Collider. (Lightning is also a pretty good particle accelerator).

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So where do cosmic rays come from? We should just be able to track them back to their source, right? Not exactly. Any time they run into a strong magnetic field on their way to Earth, they get deflected and bounce around like a game of cosmic pinball. So there’s no straight line to follow back to the source. Most of the cosmic rays from a single source don’t even make it to Earth for us to measure. They shoot off in a different direction while they’re pin balling.

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Photo courtesy of Argonne National Laboratory

In 1949 Enrico Fermi — an Italian-American physicist, pioneer of high-energy physics and Fermi satellite namesake — suggested that cosmic rays might accelerate to their incredible speeds by ricocheting around inside the magnetic fields of interstellar gas clouds. And in 2013, the Fermi satellite showed that the expanding clouds of dust and gas produced by supernovas are a source of cosmic rays.

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When a star explodes in a supernova, it produces a shock wave and rapidly expanding debris. Particles trapped by the supernova remnant magnetic field bounce around wildly.

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Every now and then, they cross the shock wave and their energy ratchets up another notch. Eventually they become energetic enough to break free of the magnetic field and zip across space at nearly the speed of light — some of the fastest-traveling matter in the universe.

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How can we track them back to supernovas when they don’t travel in a straight line, you ask? Very good question! We use something that does travel in a straight line — gamma rays (actual rays of light this time, on the more energetic end of the electromagnetic spectrum).

When the particles get across the shock wave, they interact with non-cosmic-ray particles in clouds of interstellar gas. Cosmic ray electrons produce gamma rays when they pass close to an atomic nucleus. Cosmic ray protons, on the other hand, produce gamma rays when they run into normal protons and produce another particle called a pion (Just hold on! We’re almost there!) which breaks down into two gamma rays.

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The proton- and electron-produced gamma rays are slightly different. Fermi data taken over four years showed that most of the gamma rays coming from some supernova remnants have the energy signatures of cosmic ray protons knocking into normal protons. That means supernova remnants really are powerful particle accelerators, creating a lot of the cosmic rays that we see!

There are still other cosmic ray sources on the table — like active galactic nuclei — and Fermi continues to look for them. Learn more about what Fermi’s discovered over the last 10 years and how we’re celebrating its accomplishments.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com. 

6 years ago
Think Big, Be Your Best, And Reach Out Farther Than You Can Imagine. #furtherthanbefore #pathwaytothestars

Think big, be your best, and reach out farther than you can imagine. #furtherthanbefore #pathwaytothestars #scifi #longevity #clarityofmind #health #neuroscience #physics #theoreticalphysics https://www.instagram.com/p/Bq7vZXDgX4J/?utm_source=ig_tumblr_share&igshid=aa9nsjpqc86t


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6 years ago

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Promo video put together by my wonderful spouse. Thank you, Kimmy! Join our cast of heroes as they prepare civilization to go Further than Before! #FurtherthanBefore #PathwaytotheStars #ScifiFantasy #neuroscience #physics #physiology #biotech #longevity #CRISPR #politicalscifi #strongfemalelead #strongfemalerolemodel #strongmalerolemodel #spaceopera 

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3 years ago
@shanrel @delosveronesi @woodbscinpsy-blog @sonictantra @akatsuki-deidara-katsu 

@shanrel @delosveronesi @woodbscinpsy-blog @sonictantra @akatsuki-deidara-katsu 

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6 years ago

A Much-Needed Skills, Contributions, and Direction

There are many times I ask myself, why didn’t I start a trade skill from the get-go? We can never underestimate how much it is that the people who are dedicated in these professions are a large part of that which brings a higher quality of life to all of us in one form or another. No matter what we do, if kindness and well-being are parts of our central or internal value system, humanity might…

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5 years ago
Enjoy This First-Year-Anniversary Compilation Of All Of My Works In One Title: A Cosmic Legacy: From

Enjoy this First-Year-Anniversary compilation of all of my works in one title: A Cosmic Legacy: From Earth to the Stars This title includes the following works wrapped up into one story: Further Than Before: Pathway to the Stars, Part 1 Further Than Before: Pathway to the Stars, Part 2 Pathway to the Stars: Part 1, Vesha Celeste Pathway to the Stars: Part 2, Eliza Williams Pathway to the Stars: Part 3, James Cooper Pathway to the Stars: Part 4, Universal Party Pathway to the Stars: Part 5, Amber Blythe Pathway to the Stars: Part 6, Erin Carter "Our beautiful mother world ached for a reprieve from the injustices of many, courtesy of cultures and governance systems, that forgot how to love, how to be kind, how to include others, and how to think beyond the scope of greed and power, but within the visions of shared joy and well-being." Together with the organization Eliza Williams founded, called Pathway, she and her growing team will take us on a fantastical and Utopian journey to get us out and into the farthest reaches of space. There are dilemmas such as the physiological effects of space on each of us, as well as the need for longevity and a desire to still be able to visit loved ones following long journeys. Eliza and her team develop capabilities, so we can overcome the challenges ahead and are determined to stabilize a rocky economy, wipe away suffering, violence, disease, cartels, terrorism, and trafficking in persons. They work together to tame seismic activity, weather, and fires. She and her friends tackle ways to prevent extinction and provide solutions to quality of life concerns. They even consider the longevity of our Sun and our Earth's capacity to preserve life. Eliza tackles each of these issues to get us out, and into the stars, so we can begin our biggest quest--to help our Universe breathe ever so lightly. #amazing #science #fiction #novels #best #new #books #scifi #online #read #longevity #CRISPR #physiology #neurology #physics #theoretical #philosphical #politcal #educational #STEM #AmazonAuthor #BarnesAndNobleAuthor #wellbeing #quality #biotech #nanotech #SpaceOpera #astronomy #selfpublished https://www.instagram.com/p/B2GkDbYBs0y/?igshid=ufavr7j6lsy1


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6 years ago

Easter, Spring, and April Sale!

Please support the artist; comments on Amazon, Goodreads, and Barnes & Noble are also welcome and helpful. Thank you… 🐇🐰🐣🐤🐰🐇 – – Sale throughout April on: Pathway to the Stars: Part 1, Vesha Celeste (first in booklet series) http://www.amazon.com/dp/B07J2S8LLV – –and– – Further than Before: Pathway to the Stars: Part 1 (first in novel series) http://www.amazon.com/dp/B07HL767WZ – – Quotes from series, read by…

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6 years ago
I Have Really Enjoyed My Journey On Becoming A #newly Established #scifiauthor Focusing On The #spaceopera

I have really enjoyed my journey on becoming a #newly established #scifiauthor focusing on the #spaceopera genre. I enjoy my fan base and newly created friends and acquaintances. The universe awaits us all and I thank you for your support. V/r, @matthewopdyke #theoreticalphysics #physics #biotechnology #neuroscience #nanotechnology #spacetravel https://www.instagram.com/p/BuKIV3JggkU/?utm_source=ig_tumblr_share&igshid=959w55tkryri


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matthewjopdyke - Matthew J. Opdyke
Matthew J. Opdyke

Author Matthew J. Opdyke, Science Fiction and Fantasy

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